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El paleomagnetismo. Un geodinamo del Hadeo al Paleoarqueo registrado por cristales individuales de circón
John A Tarduno1, Rory D Cottrell2, William J Davis3
1Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA. john.tarduno@rochester.edu.
Resumen
La Tierra temprana
Área de la Ciencia:
- La geofísica
- El paleomagnetismo
- Ciencias planetarias
Sus antecedentes:
- Comprender el origen de la geodinamo es crucial para la evolución de la Tierra.
- El geodinamo genera el campo magnético de la Tierra, protegiendo la atmósfera.
Objetivo del estudio:
- Para reconstruir la historia temprana del geodinamo utilizando datos de paleointensidad.
- Para investigar las condiciones necesarias para un campo geomagnético Hadeano.
Principales métodos:
- Mediciones de paleointensidad de vector completo de inclusiones magnéticas en circones de Hadeo-Arcaico.
- Análisis de los circones del conglomerado de Jack Hills, Australia Occidental.
Principales resultados:
- Los campos magnéticos registrados tienen entre 3,3 y 4,2 mil millones de años.
- Las intensidades de campo variaron entre 0,12 y 1,0 veces los valores ecuatoriales recientes.
- Pruebas de un campo geomagnético Hadeano.
Conclusiones:
- Un campo geomagnético Hadeano implica un flujo de calor superadiabático entre el núcleo y el manto.
- Sugiere la tectónica de placas temprana o el transporte de calor magmático adjetivo.
- Apoya un campo magnético previo al Bombardeo Pesado Tardío, que influye en la evolución atmosférica temprana en la Tierra y Marte.
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